Tag Archives: white

FX6 and FX9 R and B Gain values – don’t worry about the odd numbers.

I’ve noticed some users concerned or confused by the R and B gain values that they see in the cameras white balance settings after dialling in a custom white balance and tint, or after taking a white balance from a white card. The R and B gain values indicate the offset that is being applied to the Red and Blue channels relative to the Green channel and in fact they are perfectly normal. 

Typically the concern occurs when someone has used a white card to set their white balance and then these seemingly random numbers appear against the Red and Blue gain. But they are not random, they are expected, normal, and not normally something to every worry about.

The FX6 and FX9 are set up such that the indicated Red and Blue gains will only ever both be 0 when the white balance of the camera is at exactly 3200K. At any other white balance there will be an offset to the R and B gain – and that is completely normal. It is these offsets that balance the Red and Blue levels so that the white balance appears correct. At a lower colour temperature you will see a positive blue value and a negative red value. Above 3200K there will be a positive Red value and a negative Blue value.  A positive tint value will make both the Red and Blue more positive and a negative tint value will make both the Red and Blue values more negative.

All of this is perfectly normal and perfectly expected. If you have taken a white balance off a white card and then dial in a preset value you might find that the you can’t get the last  2 digits back to a zero.

For example after white balancing off a card you have 3653K but you then try to dial in 3200K, but the closest you can get is 3193K or 3213K.  This is because the smallest steps the colour temperature changes in is 20K (on the FX6 above 5640K the steps gradually get larger and larger). But this really isn’t something to worry about 3193K or 3213K are both so close to 3200K that either will do and calibration  and temperature differences will mean that the actual variations between different cameras or the camera and a colour meter will be greater than this error anyway. No two cameras will ever be truly identical and differences between lenses will cause add to this normal variation. There is no need to worry about the last 2 digits not being zero’s.

At the end of the day, these tiny differences are not something to worry or be concerned about. But if you do want to return the last digits back to zero you can do this by dialling the white balance all the way down to 2000K.

Improve the accuracy of manual white balance with the FX6 and FX9.

Have you ever struggled to get a decent white balance from a white or grey card with the Sony FX6, FX9 or in fact many other cameras (this method works equally well for the FS7, FS5, F5 and F55 etc)? Well here is a very simple trick that can really help, especially for those situations where the camera is a long way from the scene and a white card is too small in the frame for an accurate reading.

All you need to do is to cut a square hole in a piece of black card or plastic. Then when you want to take your white balance simply hold the mask in front of the lens so that it masks out the background of the shot leaving just your white card visible. It’s really simple, really easy and it really works! 

Setting The White Balance When Using The Variable ND Filter

It’s no secret that the variable ND fitted to many Sony cameras does introduce a colour shift that changes depending on how much ND you use. But the cameras are setup to add an offset to the WB as you switch the ND in or out and change the amount of ND, so in practice most people are completely unaware of this shift.
 
If you watch carefully when you engage or disengage the ND you can sometimes see a fraction of a second where the cameras electronic offset that corrects for the shift is applied just as the filter comes in. Then once the filter is in place the colours appear completely normal again.
 
So when should you white balance from a white card? With or without the ND filter in place?

You can actually white balance either with or without the ND in place. Because the camera knows exactly what offset to apply for any ND value if you change the ND it will compensate automatically and generally the compensation is very accurate. So in most cases it doesn’t really matter whether the ND filter is in place or not.
 
However, my personal recommendation is where possible to white balance with the camera setup as it will be when you are taking your footage. This should then eliminate any small errors or differences that may creep in if you do change the ND or switch the ND in or out.
 
But I wouldn’t be too concerned if you do have to do a WB at one ND level and then change the ND for whatever reason. The in camera compensation is extremely good and you would only ever really be able to see any difference if you start doing careful like for like, side by side, split screen direct comparisons. It’s certainly highly unlikely that you or your audience would ever notice any difference in normal real world applications.
 
You will often see greater colour shifts if you add external ND filters or swap between different lenses, so treat the internal ND as you would any other ND filter and WB with your lens, filters and everything else as it will be when taking the footage. I think one of the truly remarkable things about the variable ND filter is just how consistent the output of the camera is across such a wide range of ND.

Hot Pixels and White Dots From My New Camcorder (FX9 and many others).

So you have just taken delivery of a brand new PXW-FX9. Turned it on and plugged it in to a 4K TV or monitor – and shock horror there are little bright dots in the image – hot pixels.

First of all, don’t be alarmed, this is not unusual, in fact I’d actually be surprised if there weren’t any, especially if the camera has travelled in any airfreight.

Video sensors have millions of pixels and they are prone to disturbance from cosmic rays. It’s not unusual for some to become out of spec. So all modern cameras incorporate various methods of recalibrating or re-mapping those pesky problem pixels. On the Sony professional cameras this is called APR. Owners of the Sony F5, F55, Venice and FX9 will see a “Perform APR” message every couple of weeks as this is a function that needs to be performed regularly to ensure you don’t get any problems.

You should always run the APR function after flying with the camera, especially on routes over the poles as cosmic rays are greater in these areas. Also if you intend to shoot at high gain levels it is worth performing an APR run before the shoot.

If your camera doesn’t have a dedicated APR function, typically found in the maintenance section of the the camera menu system, then often the black balance function will have a very similar effect. On some Sony cameras repeatedly performing a black balance will active the APR function.

If there are a lot of problem pixels then it can take several runs of the APR routine to sort them all out. But don’t worry, it is normal and it is expected. All cameras suffer from it. Even if you have 1000 dead pixels that’s still only a teeny tiny fraction of the 19 million pixels on the sensor.

APR just takes 30 seconds or so to complete. It’s also good practice to black balance at the beginning of each day to help minimise fixed pattern noise and set the cameras black level correctly. Just remember to ensure there is a cap on the lens or camera body to exclude all outside light when you do it!

SEE ALSO: https://www.xdcam-user.com/2011/02/are-cosmic-rays-damaging-my-camera-and-flash-memory/

How to get the best White Balance (Push Auto WB).

Getting a good white balance is critical to getting a great image, especially if you are not going to be color correcting or grading your footage. When shooting traditionally ie – not with log or raw – A common way to set the cameras white balance is to use the one push auto white balance combined with a white target. You point the camera at the white target, then press the WB button (normally found at the front of the camera just under the lens).
The white target needs to occupy a good portion of the shot but it doesn’t have to completely fill the shot. It can be a pretty small area, 30% is normally enough. The key is to make sure that the white or middle grey target is obvious enough and at the right brightness that the camera uses the right part of the image for the white balance. For example, you could have a white card filling 50% of the screen, but there might be a large white car filling the rest of the shot. The camera could be confused by the car if the brightness of the car is closer to the brightness the camera wants than the white/grey card.
The way it normally works is that the camera looks for a uniformly bright part of the image with very little saturation (color) somewhere between 45 and 90IRE. The camera will then assume this area to be the white balance target. The camera then adjusts the gain of the red and blue channels so that the saturation in that part of the image becomes zero and as a result there is no color over the white or grey target.
 
If you fill the frame with your white/grey card then there can be no confusion. But that isn’t always possible or practical as the card needs to be in the scene and under the light you are balancing for rather than just directly in front of the lens. The larger your white or grey card is the more likely it is that you will get a successful and accurate white balance – provided it’s correctly exposed and in the right place.
 
The white target needs to be in reasonable focus as if it is out of focus this will create a blurred edge with color from any background objects blending into the blur. This could upset the white balance as the camera uses an average value for the whole of white area, so any color bleed at the edges due to defocussing may result in a small color offset.
 
You can use a white card or grey card (white paper at a push, but most paper is bleached slightly blue to make it look whiter to our eyes and this will offset the white balance). The best white balance is normally achieved by using a good quality photography grey card. As the grey card will be lower down in the brightness range, if there is any color, it will be more saturated. So when the camera offsets the R and B gain to eliminate the color it will be more accurate.
 
The shiny white plastic cards often sold as white balance cards are often not good choices for white balance. They are too bright and shiny. Any reflections off a glossy white card will seriously degrade the cameras ability to perform an accurate white balance as the highlights will be in the cameras knee or roll-off and as a result have much reduced saturation and also reduced R and B gain, making it harder for the camera to get a good white balance. In addition the plastics used tend to yellow with age, so if you do use a plastic white balance card make sure it isn’t past it’s best.
Don’t try to white balance off clouds or white cars, they tend to introduce offsets into the white balance.
 
Don’t read too much into the Kelvin reading the camera might give. These values are only a guide, different lenses and many other factors will introduce inaccuracies. It is not at all unusual to have two identical cameras give two different Kelvin values even though both are perfectly white balance matched. If you are not sure that your white balance is correct, repeat the process. If you keep getting the same kelvin number it’s likely you are doing it correctly.

Lastolite EzyBalance Calibration Card – Pop-up grey card and 90% white card. Review.

2014-07-15-08.35.54-300x168 Lastolite EzyBalance Calibration Card - Pop-up grey card and 90% white card. Review.
Lastolite EzyBalance pop up grey card.

Fed up with carrying large or bulky grey cards that get bent and creased or get dirty and fade? Why not try one of the great Lastolite pop up grey cards? I have the 30cm 18% grey pop-up grey card and it works really well. When folded it’s only about 12cm across so takes no space at all. It comes in a handy zip up case. This is so much easier to carry and transport than traditional ridged cards. The back of the target is 90% white. Both the grey and white targets appear to be very accurate and the matte surface of the grey card helps eliminate hot spots and reflections. There is a cross hair style focussing target in the center of each side if you need to check focus. They come in different sizes, if you want a larger one there are also 50cm and 75cm versions plus there is even an underwater version. Do note that they come in both 18% and 12% shades of grey. Really handy if shooting with SLog or for setting white balance. If you are working with a video camera you want the 18% grey version, but you may need the 12% version if calibrating a light meter etc. Simple, low cost item that works really well. Recommended!

http://www.lastolite.co.uk/ezybalance-grey-wht-card-03m-lllr1250

Whites, Super Whites and other Bits and bobs.

Do you know how your NLE is handling your video, are you whites white or whiter than white or does this sound like a washing powder add?

In the analog world you shot within the legal range of black to 100% white. It was simple, easy to understand and pretty straight forward. White was white at 100% and that was that. With digital video it all gets a lot more complicated, especially as we now start to move to greater and greater bit depths and the use of extended range recording with fancy gamma curves becomes more common. In addition computers get used more and more for not just editing but also as the final viewing device for many videos and this brings additional issues of it’s own.

First lets look at some key numbers:

8 bit data gives you 256 possible values 0 to 255.

10 bit data gives you 1024 possible values, 0 to 1023.

Computers use bit 0 to represent black and bit 255 or 1023 to represent peak white.

But video is quite different and this is where things get messy:

With 8 bit video the first 16 bits are used for sync and other data. Zero or black is always bit 16 and peak white or 100% white is always bit 235, so the traditional legal black to white range is 16 to 235, only 219 bits of data. Now in order to get a better looking image with more recording range many cameras take advantage of the bits above 235. Anything above 235 is “super white” or whiter than white in video terms, more than 100%. Cinegammas and Hypergammas take advantage of this extra range, but it’s not without it’s issues, there’s no free lunch.

10 bit video normally uses bit 64 as black and 940 as peak white. With SMPTE 10-bit extended range you can go down to bit 4 for undershoot and you can go up to bit 1019 for overshoots but the legal range is still 64-940. So black is always bit 64 and peak white always bit 940. Anything below 64 is a super black or blacker than black and anything above 940 is brighter than peak white or super white.

At the moment the big problem with 10 bit extended (SMPTE 274M 8.12) and also 8 bit that uses the extra bits above 235  is that some codecs and most software still expects to see the original legal range so anything recorded beyond that range, particularly below range can get truncated or clipped. If it is converted to RGB or you add an RGB filter or layer in your NLE it will almost certainly get clipped as the computer will take the 100% video range (16-235) and convert it to the 100% computer RGB range (0-255). So you run the risk of loosing your super whites altogether. Encoding to another codec can also lead to clipping. FCP and most NLE’s will display super blacks and super whites as these fall within the full 8 or 10 bit ranges used by computer graphics, but further encoding can be problematic as you can’t always be sure whether the conversion will use the full recorded range or just the black to white range. Baselight for example will only unpack the legal range from a codec so you need to bring the codec into legal range before going in to baselight. So as we can see it’s important to be sure that your workflow is not truncating or clipping your recorded range back to the nominal legal or 100% range.

On the other hand if you are doing stuff  where the full 0 to 255 (1023) are used then you often need to use the illegal video levels above 100% white to get whites to look white and not bright grey!  There are so many different standards across different platforms that it’s a complete nightmare. Arri with Alexa for example won’t allow you to record extanded range using ProRes because of these issues, while the Alexa HDSDi output will output extended range.

This is also an issues when using computer monitors for monitoring in the edit suite. When you look at this web page or any computer graphics white is set at bit 255 or 1023 (a lot will depend on the gamma that the monitor is set to). But that would be a super white or illegal white for video. As a result “in-range” or legal range videos when viewed on a computer monitor often look dull as the whites will be less bright than the computers own whites. The temptation therefore is to grade the video to make the whites look as bright as the computers whites which leads to illegal levels, clipping, or smply an image that does not look right on a TV or video monitor. You really need to be very careful to ensure that if you shoot using extended range that your workflow keeps that extended range intact and then you need to remember to legalise you video back to within legal range if it’s going to be broadcast.

Are Cosmic Rays Damaging my camera and flash memory?

Earth is being constantly bombarded by charged particles from outer space. Many of these cosmic rays come from exploding stars in distant galaxies. Despite being incredibly small some of these particles are travelling very fast and contain a lot of energy for their size. Every now and then one of these particles will pass through your camcorder.  What happens to both CMOS and CCD sensors as well as flash memory is that the energetic particle punches a small hole through the insulator of the pixel or memory cell. In practice what then happens is that charge can leak from the pixel to the substrate or from the substrate to the pixel. In the dark part of an image the amount of photons hitting the sensor is extremely small, each photon (in a perfect sensor) gets turn into an electron. It doesn’t take much of a leak for enough additional electrons to seep through the hole in the insulation to the pixel and give a false, bright readout. With a very small leak, the pixel may still be useable simply be adding an offset to to the read out to account for the elevated black level. In a more severe cases the pixel will be flooded with leaked electrons and appear white, in this case the masking circuits should read out the adjacent pixel.

For a computer running with big voltage/charge swings between 1’s and 0’s this small leakage current is largely inconsequential, but it does not take much to upset the readout of a sensor when your only talking of a handful of electrons. CMOS sensors are easier to mask as each pixel is addressed individually and during the camera start up it is normal to scan the sensor looking for excessively “hot” pixels. In addition many CMOS sensors incorporate pixel level noise reduction that takes a snapshot of the pixels dark voltage and subtracts it from the exposed voltage to reduce noise. A side effect of this is it masks hot pixels quite effectively. Due to the way a CCD’s output is pulled down through the entire sensor, masking is harder to do, so you often have to run a special masking routine to detect and mask hot pixels.

It may not sound much getting a single hot pixel, but if it’s right in the middle of the frame, every time that part of your scene is not brightly illuminated you see it winking away at you and on dark scenes it will stick out like a sore thumb, thankfully masking circuits are very effective at either zeroing out the raised signal level or reading out an adjacent pixel.

Flash memory can also experience these same insulation holes. There are two common types of Flash Memory, SLC and MLC. Single Level Cells have two states, on or off. Any charge means on and no charge means off. A small amount of leakage, in the short term, would have minimal impact as it could take months or years for the cell to full discharge, even then there is a 50/50 chance that the empty cell will still be giving an accurate ouput as it may have been empty to start with. Even so, long term you could loose data and a big insulation leak could discharge a cell quite quickly. MLC or Multi Level Cells are much more problematic, as the name suggests these cells can have several states, each state defined by a specific charge range, so one cell can store several bits of data. A small leak in a MLC cell can quickly alter the state of the cell form one level to the next, corrupting the data by changing the voltage.

The earths magnetic field concentrates these cosmic rays towards the north and south pole. Our atmosphere does provide some protection from them, but some of these particles can actually pass right through the earth, so lead shielding etc has no significant effect unless it is several feet thick. Your camera is at most risk when flying on polar routes. On an HD camera you can expect to have 3 or 4 pixels damaged during a year at sea level, with a CMOS camera you may never see them, with a CCD camera you may only see them with gain switched in.

SxS Pro cards (blue ones) are SLC, SxS-1 (Orange cards) use MLC as MLC works out cheaper as fewer cells are required to store the same amount of data. Most consumer flash memory is MLC. So be warned, storing data long term on flash memory may not be as safe as you might think!

The relationship between White Balance and the Matrix.

So… you want to change the look of the colour in your pictures but are not sure how to do it. One of the first things that you need to understand is the relationship between white balance and the colour matrix. They are two very different things, with two different jobs. As it’s name applies white balance is designed to ensure that whites with the image are white, even when shooting under lighting of different colour temperatures. When you shoot indoors under tungsten lights (you know, the one the EU have decided you can no longer buy) the light is very orange. When you shoot outside under sunlight the light is very blue. Our eyes adjust for this very well, so we barely notice the difference, but an electronic video camera is very sensitive to these changes. When you point a video camera at a white or grey card and do a manual white balance, what happens is that the camera adjusts the gain of the red, blue and green channels to minimise the amount of colour in areas of white (or grey) so that they do in fact appear white, ie with no colour. So the important thing to remember is that white balance is trying to eliminate colour in whites and greys.

The Matrix however deals purely with saturated parts of the image or areas where there is colour. It works be defining the ratio of how each colour is mixed with it’s complimentary colours. So changing the white balance does not alter the matrix and changing the matrix does not alter the white balance (whites will still be white). What changing the matrix will do is change the hue of the image, so you could make greens look bluer for example or reds more green.

So if you want to make your pictures look warmer (more orange or red) overall, then you would do this by offsetting the white balance, as in a warm picture your whites would appear warmer if they are slightly orange. This could be done electronically by adding an offset to the colour temperature settings or by using a warming card, which is a very slightly blue card. If you want to make the reds richer in your pictures then you would use the matrix as this allows you to make the reds stronger relative to the other colours, while whites stay white.

PDW 700 Native White Balance

The PDW-700 cameras are balanced for daylight optically and then corrected electronically for tungsten etc.

Traditionally cameras were balanced for Tungsten and then added colour correction optical filters to get to daylight. This was done as CC filters absorb light and thus make the camera less sensitive. Normally when shooting outdoors in daylight sensitivity is not an issue while shooting indoors under tungsten light you used to need every bit of sensitivity you could get.

The down side to this approach is that tungsten contains very little blue light so to get a natural picture the blue channel was often running at quite a high level of gain which increases noise in the blue channel and thus overall noise. In addition when you rotated in the CC filters to get to daylight the sensitivity of the camera was reduced, so you did not have constant gain.

With the PDW-700 (and also the F350 I believe) the cameras are essentially balanced for daylight, without the use of any CC filters, which helps reduce noise in the blue channel. Then for tungsten shooting you electronically re balance the camera. By doing this the overall sensitivity of the camera is constant whether shooting at 3.2K or 5.6K and you only get additional blue channel noise while shooting under tungsten. If you are worried by blue channel noise you can always correct from daylight down to tungsten with an optical CC filter (80A) and leave the camera set to daylight, although this will reduce the systems overall sensitivity by around 1 and a half stops.